Observations of late time acceleration of the Universe surprised the whole cosmological community [1]} . Ever since then a lot of work has been done in order to explain this expansion which include the standard ones like the Cosmological constant [1]}, [3]}, [4]}, [5]}, [6]} alongside more exotic scenarios like Modified gravity theories[7]}, [8]}, [9]}and very appealing ways of detecting dark energy directly have been put forward recently as well [10]}. An exciting approach towards understanding dark energy is that of Quintessence, where a scalar field drives the late-time cosmic acceleration of the universe[11]}, [12]}, [13]}, [14]}, [15]}, [16]}, [17]}, [18]}, [19]}, [20]}, [21]}.There has also been an expansive literature in recent times which has been devoted to the study of various types of singularities that could occur during the current and far future of the Universe with emphasis to various approaches towards dark energy [22]}, [23]}, [24]}, [25]}. These cosmological singularities which have been discussed in recent times can be classified broadly into two types ; strong and weak.
